Thermal Processing of Solids Encountering a Young Jovian Core

Jupiter's enhancement in nitrogen relative to hydrogen when compared the Sun has been interpreted as evidence that its early formation occurred beyond N$_{2}$ snowline ($\sim$ 20-40 AU). However, rapid growth necessary form Jupiter before dissipation of solar nebula would lead forming planet's core reaching very high temperatures ($>$1000 K), which it warming surroundings. Here, we explore effects a luminous planetary on solids ultimately accretes. We find critical transition occurs where hot (rapidly accreting) cores drive off volatiles prior accretion, while cool (slowly are able inherit volatile rich solids. Given enrichment, if formed snowline, could not have accreted at rate above 10$^{-10}$ M$_{\odot}$ yr$^{-1}$. Our results suggest either more distal regions nebula, or loss was suppressed, by incorporation refractory carriers because trapped within ices devolatilized higher temperatures.